Further, the statistical treatment of SNe Ia, their dimming and their ability to prove the cosmic acceleration is still a topic of debate in the literature. This is because the process of obtaining the SNe Ia observations is not trivial but requires some priors for interpretations and corrections to convert an observed-frame magnitude to a rest-frame magnitude. Examples discussed in the literature are for instance: possible evolutionary effects in SNe Ia events [1]}, [2]}, local Hubble bubble [3]}, [4]}, modified gravity [5]}, [6]}, [7]}, unclustetered sources of light attenuation [8]}, [9]}, [10]}, [11]} and the existence of Axion-Like-Particles (ALPs) arising in a wide range of well-motivated high-energy physics scenarios. All these could also lead to the dimming of SNe Ia brightness [12]}, [13]} which would eventually affect the second assumption used in the SNe Ia analysis.
